Postdoctoral Fellow at Tsinghua University

Jiaqi (Jake) Zhao 赵嘉琦

I study neutron stars and pulsars through X-ray observations, with a particular focus on millisecond pulsars in globular clusters and other compact high-energy systems.

Much of my work links individual X-ray counterparts to broader questions about compact-object populations, dense stellar environments, and how those systems are shaped over time.

Current focus X-ray studies of compact objects
Core themes MSPs, globular clusters, neutron stars
X-ray astronomy Millisecond pulsars Globular clusters
Current Work

Questions I keep coming back to

X-ray counterparts

Identifying X-ray counterparts to millisecond pulsars in crowded environments such as M5, M13, and Omega Centauri.

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Dense stellar systems

Using globular clusters as laboratories for how stellar interactions, binary evolution, and compact remnants shape pulsar populations.

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Broader neutron-star phenomena

Following questions beyond classic MSP studies, including the Galactic Center excess, magnetars, and long-period transients.

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Research Highlights

Compact objects in dense stellar systems

I combine detailed observational analysis with broader questions about how compact objects form, evolve, and cluster.

Millisecond pulsars in globular clusters

Globular clusters are ideal places to study MSP populations because their high stellar densities efficiently produce the binaries that spin neutron stars up to millisecond periods.

Much of my work focuses on building a clearer X-ray picture of these systems and relating them back to their environments.

From cluster cores to the Galactic bulge

I am interested in how compact-object studies in one environment inform another, especially when unresolved MSP populations enter the picture.

That thread naturally extends to the Galactic Center excess, magnetars, and long-period transients.

Optical and X-ray images of the globular cluster Omega Centauri

Omega Centauri as a case study

A recurring thread in my work is how X-ray observations can isolate faint compact systems in crowded cluster fields.

Optical and Chandra views of Omega Centauri show the kind of environment where those questions become concrete.

Selected Publications

Recent papers

2025 ApJ

Verification of Cas A neutron star cooling rate using Chandra HRC-S observations

A recent revisit of one of the field's best-known neutron-star cooling benchmarks using Chandra HRC-S observations.

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2023 MNRAS

A Chandra X-ray study of millisecond pulsars in Omega Centauri

An in-depth look at MSP X-ray properties in one of the most intriguing globular-cluster environments.

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2022 MNRAS

A census of X-ray millisecond pulsars in globular clusters

A population-level view of X-ray MSPs across globular clusters, connecting individual detections to the bigger picture.

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2021 MNRAS

Chandra and HST studies of six millisecond pulsars in M13

A multi-instrument study that helped lay part of the observational foundation for my later MSP work.

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Mountain landscape from Larch Valley

Beyond research

When I am away from telescope data and source catalogs, I usually end up outside. Hiking, camping, snowboarding, and long drives toward the Rockies have become an important counterweight to academic life.

The personal side of the site is still here, just with a calmer frame around it.

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